A new family of solutions has been found for force-free magnetic fields and Beltrami flows, which admits a complete classification in terms of the eigenvalues of the problem. In the absence of boundary values to determine them uniquely, the eigenvalues correspond to the entire set of real numbers, except for zero. The eigenvalues are degenerate in that each eigenvalue has many eigensolutions associated with it. For each eigensolution we have been able to identify sets of equilibrium or null points and lines. The linear mappings of these null points and lines are all unstable. Finally, we derive the first integral of energy associated with this family of solutions
Force-free electrodynamics (FFE) describes a particular regime of magnetically dominated relativisti...
Force-free magnetic fields are important in many astrophysical settings. Determining the properties ...
A generalized energy principle for finite-pressure, toroidalmagnetohydrodynamic(MHD) equilibria in g...
Incontrovertible evidence is presented that the force-free magnetic fields exhibit strong stochastic...
International audienceFor solving the nonlinear equations governing force-free fields, an iterative ...
Recently, a family of exact force-free electrodynamic (FFE) solutions was given by Brennan, Gralla a...
Force-free magnetic fields and Beltrami flows, which are selenoidal vector fields and satisfy the co...
In this paper, a theory of force-free magnetic field useful for explaining the formation of convex c...
Funding: STFC Consolidated Grant [ST/K000950/1] (OA, TN & FW) and a Doctoral Training Grant [ST/K502...
After an introductory chapter concerned with the history of force-free magnetic fields, and the rela...
Beltrami fields, eigen functions of the curl operator, represent the static force-free relaxed state...
Solenoidal vector fields, which satisfy the condition that the field vector everywhere parallels to ...
Beltrami fields, eigen functions of the curl operator, represent the static force-free relaxed state...
Electromagnetic field configurations with vanishing Lorentz force density are known as force-free an...
Plasma-filled magnetospheres can extract energy from a spinning black hole and provide the power sou...
Force-free electrodynamics (FFE) describes a particular regime of magnetically dominated relativisti...
Force-free magnetic fields are important in many astrophysical settings. Determining the properties ...
A generalized energy principle for finite-pressure, toroidalmagnetohydrodynamic(MHD) equilibria in g...
Incontrovertible evidence is presented that the force-free magnetic fields exhibit strong stochastic...
International audienceFor solving the nonlinear equations governing force-free fields, an iterative ...
Recently, a family of exact force-free electrodynamic (FFE) solutions was given by Brennan, Gralla a...
Force-free magnetic fields and Beltrami flows, which are selenoidal vector fields and satisfy the co...
In this paper, a theory of force-free magnetic field useful for explaining the formation of convex c...
Funding: STFC Consolidated Grant [ST/K000950/1] (OA, TN & FW) and a Doctoral Training Grant [ST/K502...
After an introductory chapter concerned with the history of force-free magnetic fields, and the rela...
Beltrami fields, eigen functions of the curl operator, represent the static force-free relaxed state...
Solenoidal vector fields, which satisfy the condition that the field vector everywhere parallels to ...
Beltrami fields, eigen functions of the curl operator, represent the static force-free relaxed state...
Electromagnetic field configurations with vanishing Lorentz force density are known as force-free an...
Plasma-filled magnetospheres can extract energy from a spinning black hole and provide the power sou...
Force-free electrodynamics (FFE) describes a particular regime of magnetically dominated relativisti...
Force-free magnetic fields are important in many astrophysical settings. Determining the properties ...
A generalized energy principle for finite-pressure, toroidalmagnetohydrodynamic(MHD) equilibria in g...